* Astronomy

Title: A very bright i=16.44 quasar in the 'redshift desert' discovered by LAMOST
Authors: Xue-Bing Wu, Zhaoyu Chen, Zhendong Jia, Wenwen Zuo, Yongheng Zhao, Ali Luo, Zhongrui Bai, Jianjun Chen, Haotong Zhang, Hongliang Yan, Juanjuan Ren, Shiwei Sun, Hong Wu, Yong Zhang, Yeping Li, Qishuai Lu, You Wang, Jijun Ni, Hai Wang, Xu Kong, Shiyin Shen

The redshift range from 2.2 to 3, is known as the 'redshift desert' of quasars because quasars with redshift in this range have similar optical colours as normal stars and are thus difficult to be found in optical sky surveys. A quasar candidate, SDSS J085543.40-001517.7, which was selected by a recently proposed criterion involving near-IR Y-K and optical g-z colours, was identified spectroscopically as a new quasar with redshift of 2.427 by the LAMOST commissioning observation in December 2009 and confirmed by the observation made with the NAOC/Xinglong 2.16m telescope in March 2010. This quasar was not targeted in the SDSS spectroscopic survey because it locates in the stellar locus of the optical colour-colour diagrams, while it is clearly separated from stars in the Y-K vs. g-z diagram. Comparing with other SDSS quasars we found this new quasar with i magnitude of 16.44 is apparently the brightest one in the redshift range from 2.3 to 2.7. From the spectral properties we derived its central black hole mass as (1.4 ~3.9) x 10^{10} solar masses and the bolometric luminosity as 3.7 x  10^{48} \ergs, which indicates that this new quasar is intrinsically very bright and belongs to the most luminous quasars in the universe. Our identification supports that quasars in the redshift desert can be found by the quasar selection criterion involving the near-IR colours. More missing quasars are expected to be recovered by the future LAMOST spectroscopic surveys, which is important to the study of the cosmological evolution of quasars at redshift higher than 2.2.

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